INTEGRAL Galactic bulge Monitoring
Revolution 1209: Observation start 2012-09-08T01:37 = MJD 56178.068
Total Observation GTI = 15896 seconds
IBIS/ISGRI
IBIS/ISGRI significance mosaic images. Left: IBIS/ISGRI 18-40 keV. Right: 40-100 keV
Sources detected > 10σ in each band are marked on the image. The table below lists the fitted position, and statistical positional uncertainty in arcmin returned by the mosaic step of
OSA10.1, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 208 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 100 cps ) where available.NOTES: The table is constructed from the
isgri_mosa_res.fits file - fluxes in the mosaic output are known to be systematically ~10% lower than in the ScW light-curves (see known issues). The systematic noise increases towards the edge of the field of view and NEW SOURCEs < 6σ towards the border of the image may be spurious. IBIS/ISGRI Detected Sources 18-40 keV (A) and 40-100 keV (B)
Source Name RA dec +/- l b A(cps) +/- sig B(cps) +/- sig ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== 4U 1700-377 255.988 -37.850 0.4 347.750 +2.169 79.9 0.69 116.6 26.2 0.45 57.7 GX 5-1 270.277 -25.080 0.9 5.073 -1.013 10.9 0.29 37.3 0.0 0.00 0.0 Ginga 1826-24 277.354 -23.793 1.1 9.270 -6.075 13.5 0.51 26.4 5.7 0.35 16.3 GRS 1758-258 270.299 -25.732 1.1 4.516 -1.353 7.7 0.29 26.5 5.1 0.21 24.5 1E 1740.7-2942 266.017 -29.770 1.8 359.112 -0.147 5.3 0.33 15.9 2.8 0.25 11.4 GX 349+2 256.499 -36.431 2.0 349.128 +2.703 8.2 0.58 14.1 0.0 0.00 0.0 H 1820-303 275.932 -30.368 1.9 2.787 -7.927 5.9 0.41 14.6 0.0 0.00 0.0 GX 354-0 262.992 -33.849 1.9 354.291 -0.160 5.4 0.36 15.0 1.9 0.25 7.7 GX 1+4 262.996 -24.765 2.0 1.914 +4.795 4.5 0.32 14.1 0.0 0.00 0.0 OAO 1657-415 255.236 -41.642 3.4 344.395 +0.309 13.5 1.79 7.6 0.0 0.00 0.0 4U 1722-30 261.905 -30.808 2.9 356.323 +2.283 3.0 0.34 8.9 1.0 0.24 4.3 GX 3+1 266.980 -26.587 3.1 2.272 +0.784 2.5 0.30 8.4 0.0 0.00 0.0 GX 9+1 270.375 -20.526 3.4 9.075 +1.163 3.2 0.41 7.7 0.0 0.00 0.0 IGR J17091-3624 257.176 -36.362 3.1 349.510 +2.307 4.6 0.55 8.5 3.2 0.37 8.6 3A 1822-371 276.431 -37.140 3.7 356.813 -11.296 4.2 0.60 6.9 0.0 0.00 0.0 SLX 1735-269 264.589 -26.957 4.4 0.836 +2.407 1.7 0.00 5.8 1.0 0.22 4.6 V2400 Oph 258.191 -24.243 4.2 359.890 +8.712 2.7 0.45 6.0 0.0 0.00 0.0 XTE J1739-285 265.025 -28.556 4.4 359.687 +1.229 1.8 0.32 5.6 0.0 0.00 0.0 1RXS J165424.7-29541 253.632 -29.959 5.6 352.803 +8.556 2.8 0.65 4.4 0.0 0.00 0.0 1H 1746-370 267.571 -37.032 5.1 353.556 -5.007 2.1 0.44 4.9 0.0 0.00 0.0 SGR J1745-29 266.524 -29.028 0.0 359.975 -0.137 1.3 0.00 4.1 0.0 0.00 0.0 XTE J1807-294 271.799 -29.462 6.1 1.909 -4.336 1.3 0.32 4.0 0.0 0.00 0.0
JEM-X
JEM-X1+2 combined significance mosaic images. Left: 3-10 keV. Right: 10-25 keV.
Sources labelled were detected in the 3-10 keV image > 6σ. The sources detected above 3σ in the 3-10 keV and/or 10-25 keV band are listed in the table below. Fluxes are extracted at the known catalogue position of the source (i.e. no fitting of the source position is done), with
mosaic_spec, in two bands: A = 3-10 keV (1 Crab ~ 97 cps [J1], 103 cps [J2]); B = 10-25 keV (1 Crab ~ 29 cps [J1], 27 cps [J2]). NOTES: The object marked as SLX 1744-299_300 is used to indicate two low-mass x-ray binaries separated by 2.7 arcminutes, SLX 1744-299 and SLX 1744-300; the position for SLX 1744-299 is used, although it can not be ruled out that SLX 1744-300 may dominate the emission some of the time. The systematic noise increases towards the edge of the field of view and in the vicinity of very bright sources, such as GX 5-1;
NEW SOURCEs < 6σ towards the border of the image and/or near GX 5-1 may, therefore, be spurious.
JEM-X1+2 Detected Sources in 3-10 keV (A) and 10-25 keV (B).
Source Name RA dec l b A(cps) +/- sig B(cps) +/- sig ==================== ======== ======= ======== ======== ====== ===== ===== ====== ===== ===== 1A 1742-294 266.523 -29.515 359.559 -0.389 8.3 0.23 35.9 1.3 0.12 11.2 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.3 0.23 10.3 0.9 0.12 7.5 4U 1722-30 261.888 -30.802 356.320 +2.298 3.7 0.53 7.0 0.9 0.34 2.7 GRS 1734-292 264.367 -29.142 358.883 +1.404 1.3 0.25 5.5 0.2 0.13 1.5 GRS 1758-258 270.303 -25.741 4.511 -1.361 1.5 0.67 2.2 1.0 0.30 3.2 GX 3+1 266.985 -26.566 2.293 +0.791 56.6 0.33 172.6 6.2 0.15 42.2 GX 5-1 270.283 -25.065 5.089 -1.011 126.8 0.99 128.0 15.5 0.44 35.6 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.7 0.23 7.2 0.5 0.12 3.8 XTE J1739-285 264.975 -28.496 359.714 +1.298 10.7 0.24 44.1 1.2 0.12 9.9 NEW SOURCE 266.285 -28.996 359.894 +0.058 1.6 0.22 7.4 0.2 0.11 1.5 NEW SOURCE 269.885 -24.597 5.316 -0.465 6.0 0.97 6.1 1.2 0.47 2.5 NEW SOURCE 267.171 -24.269 4.348 +1.832 3.6 0.63 5.7 0.5 0.31 1.6 NEW SOURCE 271.906 -24.604 6.213 -2.069 12.0 2.16 5.6 2.5 1.22 2.0 NEW SOURCE 269.113 -27.744 2.244 -1.439 1.6 0.30 5.4 0.2 0.14 1.1 NEW SOURCE 272.814 -26.178 5.228 -3.546 10.0 1.73 5.8 1.4 0.98 1.4 Swift J174444.9-2950 266.193 -29.847 359.126 -0.318 0.0 0.00 0.0 0.5 0.12 3.8 NEW SOURCE 269.854 -24.616 5.285 -0.449 4.6 0.96 4.8 1.4 0.46 3.0